Magnetic Reconnection Triggered by the Parker Instability in the Galaxy: Two‐dimensional Numerical Magnetohydrodynamic Simulations and Application to the Origin of X‐Ray Gas in the Galactic Halo | Zendy

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Magnetic Reconnection Triggered by the Parker Instability in the Galaxy: Two‐dimensional Numerical Magnetohydrodynamic Simulations and Application to the Origin of X‐Ray Gas in the Galactic Halo

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